Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29527
DC Field | Value | Language |
---|---|---|
dc.contributor.author | EVANGELISTA, YURI | en_US |
dc.contributor.author | AMBROSINO, Filippo | en_US |
dc.contributor.author | FEROCI, MARCO | en_US |
dc.contributor.author | Bellutti, P. | en_US |
dc.contributor.author | Bertuccio, G. | en_US |
dc.contributor.author | Borghi, G. | en_US |
dc.contributor.author | CAMPANA, RICCARDO | en_US |
dc.contributor.author | Caselle, M. | en_US |
dc.contributor.author | Cirrincione, D. | en_US |
dc.contributor.author | Ficorella, F. | en_US |
dc.contributor.author | FIORINI, MAURO | en_US |
dc.contributor.author | FUSCHINO, FABIO | en_US |
dc.contributor.author | Gandola, M. | en_US |
dc.contributor.author | Grassi, M. | en_US |
dc.contributor.author | LABANTI, CLAUDIO | en_US |
dc.contributor.author | Malcovati, P. | en_US |
dc.contributor.author | Mele, F. | en_US |
dc.contributor.author | MORBIDINI, Alfredo | en_US |
dc.contributor.author | Picciotto, A. | en_US |
dc.contributor.author | Rachevski, A. | en_US |
dc.contributor.author | Rashevskaya, I. | en_US |
dc.contributor.author | Sammartini, M. | en_US |
dc.contributor.author | Zampa, G. | en_US |
dc.contributor.author | Zampa, N. | en_US |
dc.contributor.author | Zorzi, N. | en_US |
dc.contributor.author | Vacchi, A. | en_US |
dc.date.accessioned | 2021-01-07T11:38:55Z | - |
dc.date.available | 2021-01-07T11:38:55Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 1748-0221 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29527 | - |
dc.description.abstract | Multi-pixel fast silicon detectors represent the enabling technology for the next generation of space-borne experiments devoted to high-resolution spectral-timing studies of low-flux compact cosmic sources. Several imaging detectors based on frame-integration have been developed as focal plane devices for X-ray space-borne missions but, when coupled to large-area concentrator X-ray optics, these detectors are affected by strong pile-up and dead-time effects, thus limiting the time and energy resolution as well as the overall system sensitivity. The current technological gap in the capability to realize pixelated silicon detectors for soft X-rays with fast, photon-by-photon response and nearly Fano-limited energy resolution therefore translates into the unavailability of sparse read-out sensors suitable for high throughput X-ray astronomy applications. In the framework of the ReDSoX Italian collaboration, we developed a new, sparse read-out, pixelated silicon drift detector which operates in the energy range 0.5-15 keV with nearly Fano-limited energy resolution (<=150 eV FWHM @ 6 keV) at room temperature or with moderate cooling (~0°C to +20°C). In this paper, we present the design and the laboratory characterization of the first 16-pixel (4 × 4) drift detector prototype (PixDD), read-out by individual ultra low-noise charge sensitive preamplifiers (SIRIO) and we discuss the future PixDD prototype developments. | en_US |
dc.language.iso | eng | en_US |
dc.title | Characterization of a novel pixelated Silicon Drift Detector (PixDD) for high-throughput X-ray astrophysics | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1088/1748-0221/13/09/P09011 | en_US |
dc.identifier.scopus | 2-s2.0-85055577626 | en_US |
dc.identifier.isi | 000444645300003 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.1088/1748-0221/13/09/P09011 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 13 | en_US |
dc.relation.issue | 9 | en_US |
dc.relation.firstpage | P09011 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | DEU | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | JOURNAL OF INSTRUMENTATION | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018JInst..13P9011E | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0001-6096-6710 | - |
crisitem.author.orcid | 0000-0001-7915-996X | - |
crisitem.author.orcid | 0000-0002-7617-3421 | - |
crisitem.author.orcid | 0000-0002-4794-5453 | - |
crisitem.author.orcid | 0000-0001-8297-1983 | - |
crisitem.author.orcid | 0000-0003-2139-3299 | - |
crisitem.author.orcid | 0000-0002-5086-3619 | - |
crisitem.author.orcid | 0000-0002-4189-4616 | - |
crisitem.journal.journalissn | 1748-0221 | - |
crisitem.journal.ance | E190325 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1808.08041.pdf | postprint | 11.09 MB | Adobe PDF | View/Open |
Evangelista_2018_J._Inst._13_P09011.pdf | [Administrators only] | 11.5 MB | Adobe PDF | |
29527-Evangelista_2018_J._Inst._13_P09011_P01.pdf | Miur | 9.62 MB | Adobe PDF | |
29527-Evangelista_2018_J._Inst._13_P09011_P02.pdf | Miur | 2.03 MB | Adobe PDF |
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